A MAGNETIC RIBBON MODEL for STAR-FORMING FILAMENTSSayantan Auddy, Takahiro Kudoh, Shantanu Basu|Scholarship@Western (Western University)|2016Cited by 25
The effect of magnetic fields and ambipolar diffusion on the column density probability distribution function in molecular cloudsSayantan Auddy, Takahiro Kudoh, Shantanu Basu|Monthly Notices of the Royal Astronomical Society|2017Cited by 16
The Transition from a Lognormal to a Power-law Column Density Distribution in Molecular Clouds: An Imprint of the Initial Magnetic Field and TurbulenceSayantan Auddy, Takahiro Kudoh, Shantanu Basu|The Astrophysical Journal Letters|2019Cited by 6
The Magnetic Field versus Density Relation in Star-forming Molecular CloudsSayantan Auddy, Takahiro Kudoh, Shantanu Basu|The Astrophysical Journal Letters|2022Cited by 6
Magnetic Ribbons: A Minimum Hypothesis Model for FilamentsSayantan Auddy, Takahiro Kudoh, Shantanu Basu|arXiv (Cornell University)|2017Cited by 1